Generation of resonance transition emissions in the solar atmosphere

Gregory Fleishman

doi:10.1134/1.1358383

Generation of resonance transition emissions in the solar atmosphere

Gregory Fleishman

Center For Solar Terrestrial Research - Big Bear Solar Observatory

Research output: Contribution to journal › Article › peer-review

13 Scopus citations

Abstract

We derive formulas for the radio flux generated in solar flares by the resonance transition mechanism. This mechanism is shown to produce the observed decimeter-wave emission in continuum radio bursts at a level of small-scale irregularities of ∼10^-6-10^-7. Thus, an analysis of continuum decimeter emission offers a unique opportunity to study small-scale turbulence in solar flares.

Original language	English (US)
Pages (from-to)	254-259
Number of pages	6
Journal	Astronomy Letters
Volume	27
Issue number	4
DOIs	https://doi.org/10.1134/1.1358383
State	Published - Apr 2001

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Keywords

Plasma diagnostics
Small-scale turbulence
Solar flares

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10.1134/1.1358383

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title = "Generation of resonance transition emissions in the solar atmosphere",

abstract = "We derive formulas for the radio flux generated in solar flares by the resonance transition mechanism. This mechanism is shown to produce the observed decimeter-wave emission in continuum radio bursts at a level of small-scale irregularities of ∼10-6-10-7. Thus, an analysis of continuum decimeter emission offers a unique opportunity to study small-scale turbulence in solar flares.",

keywords = "Plasma diagnostics, Small-scale turbulence, Solar flares",

author = "Gregory Fleishman",

note = "Funding Information: ACKNOWLEDGMENTS I am grateful to V.F. Mel{\textquoteright}nikov for a helpful discussion. The work was supported in part by the Russian Foundation for Basic Research (project no. 00-02-16356).",

year = "2001",

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doi = "10.1134/1.1358383",

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volume = "27",

pages = "254--259",

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T1 - Generation of resonance transition emissions in the solar atmosphere

AU - Fleishman, Gregory

N1 - Funding Information: ACKNOWLEDGMENTS I am grateful to V.F. Mel’nikov for a helpful discussion. The work was supported in part by the Russian Foundation for Basic Research (project no. 00-02-16356).

PY - 2001/4

Y1 - 2001/4

N2 - We derive formulas for the radio flux generated in solar flares by the resonance transition mechanism. This mechanism is shown to produce the observed decimeter-wave emission in continuum radio bursts at a level of small-scale irregularities of ∼10-6-10-7. Thus, an analysis of continuum decimeter emission offers a unique opportunity to study small-scale turbulence in solar flares.

AB - We derive formulas for the radio flux generated in solar flares by the resonance transition mechanism. This mechanism is shown to produce the observed decimeter-wave emission in continuum radio bursts at a level of small-scale irregularities of ∼10-6-10-7. Thus, an analysis of continuum decimeter emission offers a unique opportunity to study small-scale turbulence in solar flares.

KW - Plasma diagnostics

KW - Small-scale turbulence

KW - Solar flares

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SP - 254

EP - 259

JO - Astronomy Letters

JF - Astronomy Letters

IS - 4

ER -

Generation of resonance transition emissions in the solar atmosphere

Abstract

All Science Journal Classification (ASJC) codes

Keywords

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